Ay. Drobysh et Vm. Ostryakov, THE INFLUENCE OF MHD TURBULENCE ON THE STABILITY OF A TANGENTIAL DISCONTINUITY, Astronomy reports, 42(5), 1998, pp. 679-687
The stability conditions for a tangential discontinuity in a turbulent
medium are obtained on the basis of ideal magnetohydrodynamic equatio
ns. The turbulence is represented as a high-frequency, short-wavelengt
h background with respect to the mean parameter values and coherent pe
rturbations. The two cases of weakly and strongly compressible plasma
are analyzed in detail. In the former case, anisotropic turbulence can
result in the stabilization of a tangential discontinuity. The analog
y of this limiting case with the firehose instability in an anisotropi
c plasma is noted. In a strongly compressible (clumpy) medium, the tur
bulence is a destabilizing factor, though new stable directions in the
propagation of the perturbation appear (in comparison with the lamina
r case). Instability increments for discontinuities in the interplanet
ary medium are estimated.